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Search Results (12,107)

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Keywords = optical measurement

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35 pages, 7517 KiB  
Review
Recent Advances in Applications of Ultrafast Lasers
by Sibo Niu, Wenwen Wang, Pan Liu, Yiheng Zhang, Xiaoming Zhao, Jibo Li, Maosen Xiao, Yuzhi Wang, Jing Li and Xiaopeng Shao
Photonics 2024, 11(9), 857; https://doi.org/10.3390/photonics11090857 (registering DOI) - 11 Sep 2024
Abstract
Ultrafast lasers, characterized by femtosecond and picosecond pulse durations, have revolutionized material processing due to their high energy density and minimal thermal diffusion, and have played a transformative role in precision manufacturing. This review first traces the progression from early ruby lasers to [...] Read more.
Ultrafast lasers, characterized by femtosecond and picosecond pulse durations, have revolutionized material processing due to their high energy density and minimal thermal diffusion, and have played a transformative role in precision manufacturing. This review first traces the progression from early ruby lasers to modern titanium–sapphire lasers, highlighting breakthroughs like Kerr-lens mode-locking and chirped pulse amplification. It also examines the interaction mechanisms between ultrafast pulses and various materials, including metals, dielectrics, and semiconductors. Applications of ultrafast lasers in microstructure processing techniques are detailed, such as drilling, cutting, surface ablation, and nano welding, demonstrating the versatility and precision of the technology. Additionally, it covers femtosecond laser direct writing for optical waveguides and the significant advancements in imaging and precision measurement. This review concludes by discussing potential future advancements and industrial applications of ultrafast lasers. Full article
(This article belongs to the Special Issue New Perspectives in Ultrafast Intense Laser Science and Technology)
19 pages, 22517 KiB  
Article
Development of a High-Precision Deep-Sea Magnetic Survey System for Human-Occupied Vehicles
by Qimao Zhang, Keyu Zhou, Ming Deng, Qisheng Zhang, Yongqiang Feng and Leisong Liu
Electronics 2024, 13(18), 3611; https://doi.org/10.3390/electronics13183611 - 11 Sep 2024
Abstract
The high-precision magnetic survey system is crucial for ocean exploration. However, most existing systems face challenges such as high noise levels, low sensitivity, and inadequate magnetic compensation effects. To address these issues, we developed a high-precision magnetic survey system based on the manned [...] Read more.
The high-precision magnetic survey system is crucial for ocean exploration. However, most existing systems face challenges such as high noise levels, low sensitivity, and inadequate magnetic compensation effects. To address these issues, we developed a high-precision magnetic survey system based on the manned submersible “Deep Sea Warrior” for deep-ocean magnetic exploration. This system incorporates a compact optically pumped cesium (Cs) magnetometer sensor to measure the total strength of the external magnetic field. Additionally, a magnetic compensation sensor is included at the front end to measure real-time attitude changes of the platform. The measured data are then transmitted to a magnetic signal processor, where an algorithm compensates for the platform’s magnetic interference. We also designed a deep pressure chamber to allow for a maximum working depth of 4500 m. Experiments conducted in both indoor and field environments verified the performance of the proposed magnetic survey system. The results showed that the system’s sensitivity is ≤0.5 nT, the noise level of the magnetometer sensor is ≤1 pT/√Hz at 1 Hz, and the sampling rate is 10 Hz. The proposed system has potential applications in ocean and geophysical exploration. Full article
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Figure 1
<p>Overall architecture of the human-occupied, vehicular platform-based, high-precision, deep-sea magnetic survey system.</p>
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<p>Design of the optically pumped magnetometer sensor.</p>
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<p>Block diagram of the optically pumped magnetometer sensor circuitry.</p>
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<p>Structure of the fluxgate sensor.</p>
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<p>3D model diagram of fluxgate sensor.</p>
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<p>Block diagram of the magnetic compensation circuitry.</p>
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<p>Power management circuit diagram.</p>
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<p>Schematic of waveform generation circuit.</p>
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<p>Block diagram of the magnetic signal processor.</p>
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<p>Functional modules of the magnetic signal processing software.</p>
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<p>Data processing flowchart using the magnetic signal processing software.</p>
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<p>Functional modules of the display and control software.</p>
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<p>User interface of the display and control software.</p>
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<p>3D model of pressure chamber. (<b>a</b>) Electronic pressure chamber. (<b>b</b>) Assembly of the probe pressure chamber.</p>
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<p>Actual manned submersible sampling basket.</p>
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<p>Assembly position of the magnetometer equipment.</p>
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<p>Noise test scenario.</p>
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<p>Noise level spectrum.</p>
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<p>Anti-aliasing filtering and re-sampling process.</p>
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<p>Alternating magnetic field test result.</p>
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<p>The noise levels of compensated magnetic field signals before and after geomagnetic gradient correction.</p>
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<p>Flight trajectory for calibrating magnetic noise compensation.</p>
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<p>Compensation performance before and after calibration flight trial.</p>
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<p>Fluxgate spectrum for the magnetic compensation actions.</p>
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16 pages, 1117 KiB  
Article
Machine Learning-Based Retrieval of Total Ozone Column Amount and Cloud Optical Depth from Irradiance Measurements
by Milos Sztipanov, Levente Krizsán, Wei Li, Jakob J. Stamnes, Tove Svendby and Knut Stamnes
Atmosphere 2024, 15(9), 1103; https://doi.org/10.3390/atmos15091103 - 11 Sep 2024
Viewed by 86
Abstract
A machine learning algorithm combined with measurements obtained by a NILU-UV irradiance meter enables the determination of total ozone column (TOC) amount and cloud optical depth (COD). In the New York City area, a NILU-UV instrument on the rooftop of a Stevens Institute [...] Read more.
A machine learning algorithm combined with measurements obtained by a NILU-UV irradiance meter enables the determination of total ozone column (TOC) amount and cloud optical depth (COD). In the New York City area, a NILU-UV instrument on the rooftop of a Stevens Institute of Technology building (40.74° N, −74.03° E) has been used to collect data for several years. Inspired by a previous study [Opt. Express 22, 19595 (2014)], this research presents an updated neural-network-based method for TOC and COD retrievals. This method provides reliable results under heavy cloud conditions, and a convenient algorithm for the simultaneous retrieval of TOC and COD values. The TOC values are presented for 2014–2023, and both were compared with results obtained using the look-up table (LUT) method and measurements by the Ozone Monitoring Instrument (OMI), deployed on NASA’s AURA satellite. COD results are also provided. Full article
(This article belongs to the Section Atmospheric Techniques, Instruments, and Modeling)
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Figure 1
<p>The absolute spectral response of No. 115 NILU-UV instrument.</p>
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<p>Cloud optical depth <math display="inline"><semantics> <mrow> <msub> <mi>τ</mi> <mi>c</mi> </msub> <mstyle scriptlevel="1" displaystyle="false"> <mrow> <mo>(</mo> <mn>380</mn> <mspace width="0.166667em"/> <mi>nm</mi> <mo>)</mo> </mrow> </mstyle> </mrow> </semantics></math> versus cloud volume fraction <math display="inline"><semantics> <msub> <mi>f</mi> <mrow> <mi>V</mi> <mo>,</mo> <mi>c</mi> </mrow> </msub> </semantics></math>.</p>
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<p>Modeled relation between RMF and <math display="inline"><semantics> <mrow> <msub> <mi>τ</mi> <mi>c</mi> </msub> <mstyle scriptlevel="1" displaystyle="false"> <mrow> <mo>(</mo> <mn>380</mn> <mspace width="0.166667em"/> <mi>nm</mi> <mo>)</mo> </mrow> </mstyle> </mrow> </semantics></math>.</p>
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<p>Cloud volume fraction results by the MLNN vs. modeled values.</p>
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<p>Scaled TOC by the MLNN vs. the modeled values.</p>
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<p>Schematic illustration of the retrieval methodology.</p>
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<p>TOC amounts from OMI (gray dots) and NILU-UV (black crosses) versus day of the year for (<b>a</b>): 2014; (<b>b</b>): 2015; (<b>c</b>): 2018; and (<b>d</b>): 2019.</p>
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<p>The seasonal variations in TOC amounts: blue: winter, pink: spring, green: summer, yellow: autumn.</p>
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<p>Annual average TOC amounts from merged NILU-UV and OMI data for 2014–2023.</p>
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<p>Daily mean COD (<math display="inline"><semantics> <mrow> <msub> <mi>τ</mi> <mi>c</mi> </msub> <mstyle scriptlevel="1" displaystyle="false"> <mrow> <mo>(</mo> <mn>380</mn> <mspace width="0.166667em"/> <mi>nm</mi> <mo>)</mo> </mrow> </mstyle> </mrow> </semantics></math>) values for (<b>a</b>) 2014, (<b>b</b>) 2015, (<b>c</b>) 2018 and (<b>d</b>) 2019.</p>
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<p>TOC values from OMI (gray dots) and NILU-UV (black crosses) versus day of the year for 2016.</p>
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<p>TOC values from OMI (gray dots) and NILU-UV (black crosses) versus day of the year for 2017.</p>
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<p>Daily mean <math display="inline"><semantics> <mrow> <msub> <mi>τ</mi> <mi>c</mi> </msub> <mstyle scriptlevel="1" displaystyle="false"> <mrow> <mo>(</mo> <mn>380</mn> <mspace width="0.166667em"/> <mi>nm</mi> <mo>)</mo> </mrow> </mstyle> </mrow> </semantics></math> values versus day of the year for 2016.</p>
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<p>Daily mean <math display="inline"><semantics> <mrow> <msub> <mi>τ</mi> <mi>c</mi> </msub> <mstyle scriptlevel="1" displaystyle="false"> <mrow> <mo>(</mo> <mn>380</mn> <mspace width="0.166667em"/> <mi>nm</mi> <mo>)</mo> </mrow> </mstyle> </mrow> </semantics></math> values versus day of the year for 2017.</p>
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<p>The cosine response functions of the NILU-UV 115 instrument’s channels.</p>
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12 pages, 2862 KiB  
Article
Low-Cost, High-Efficiency Aluminum Zinc Oxide Synaptic Transistors: Blue LED Stimulation for Enhanced Neuromorphic Computing Applications
by Namgyu Lee, Pavan Pujar and Seongin Hong
Biomimetics 2024, 9(9), 547; https://doi.org/10.3390/biomimetics9090547 - 11 Sep 2024
Viewed by 152
Abstract
Neuromorphic devices are electronic devices that mimic the information processing methods of neurons and synapses, enabling them to perform multiple tasks simultaneously with low power consumption and exhibit learning ability. However, their large-scale production and efficient operation remain a challenge. Herein, we fabricated [...] Read more.
Neuromorphic devices are electronic devices that mimic the information processing methods of neurons and synapses, enabling them to perform multiple tasks simultaneously with low power consumption and exhibit learning ability. However, their large-scale production and efficient operation remain a challenge. Herein, we fabricated an aluminum-doped zinc oxide (AZO) synaptic transistor via solution-based spin-coating. The transistor is characterized by low production costs and high performance. It demonstrates high responsiveness under UV laser illumination. In addition, it exhibits effective synaptic behaviors under blue LED illumination, indicating high-efficiency operation. The paired-pulse facilitation (PPF) index measured from optical stimulus modulation was 179.6%, indicating strong synaptic connectivity and effective neural communication and processing. Furthermore, by modulating the blue LED light pulse frequency, an excitatory postsynaptic current gain of 4.3 was achieved, demonstrating efficient neuromorphic functionality. This study shows that AZO synaptic transistors are promising candidates for artificial synaptic devices. Full article
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Figure 1
<p>Schematic of the AZO synaptic transistor manufacturing method.</p>
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<p>AFM images of the surfaces of (<b>a</b>) 1-, (<b>b</b>) 3-, and (<b>c</b>) 5-layer AZO. The inset in (<b>c</b>) shows an enlarged image (1 µm × 1 μm). The values in the images are the average and RMS roughness. <span class="html-italic">I</span>–<span class="html-italic">V</span> curves of (<b>d</b>) 1-, (<b>e</b>) 3-, and (<b>f</b>) 5-layer AZO devices.</p>
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<p>(<b>a</b>) Schematic of biological synapses and neural signal transmission in neurons and the AZO synaptic transistor, which mimics neural signal transmission in neurons. (<b>b</b>) Optical microscope image of the AZO synaptic transistor. (<b>c</b>) High-resolution O 1s spectrum of AZO, showing lattice oxygen, oxygen vacancies, and alkoxide impurities. (<b>d</b>) X-ray diffraction patterns of the thin films showing the amorphous nature of AZO.</p>
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<p>(<b>a</b>) Transfer curves of the 5-layer AZO synaptic transistor measured at drain voltages of 1, 3, and 5 V. (<b>b</b>) Output curves measured at gate voltages ranging from 0 to 70 V in 15 steps (5 V increments). (<b>c</b>) Forward-sweep transfer curves at a drain voltage of 1 V under dark and irradiation conditions. The incident power densities (<span class="html-italic">P</span><sub>inc</sub>) of the UV light source were 0.1, 0.2, and 0.3 mW/cm<sup>2</sup>.</p>
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<p>(<b>a</b>) Short-term potentiation (STP) to long-term potentiation (LTP) transition in the 5-layer AZO synaptic transistor with increasing <span class="html-italic">P</span><sub>inc</sub> (λ<sub>ex</sub> = 406 nm, period (<span class="html-italic">T</span>) = 3 s, <span class="html-italic">V</span><sub>gs</sub> = 0 V, and <span class="html-italic">V</span><sub>ds</sub> = 10 V). (<b>b</b>) Variation in the excitatory postsynaptic current (EPSC) of the synaptic transistor with gate bias conditions (<span class="html-italic">T</span> = 5 s and <span class="html-italic">P</span><sub>inc</sub> = 0.3 mW/cm<sup>2</sup>). (<b>c</b>) EPSC modulation under different drain bias conditions at a pair of optical pulses (<span class="html-italic">T</span> = 1 s, <span class="html-italic">P</span><sub>inc</sub> = 0.1 mW/cm<sup>2</sup> and <span class="html-italic">V</span><sub>gs</sub> = 0 V). The inset shows the modulation ar <span class="html-italic">V</span><sub>ds</sub> = 0.1 V. (<b>d</b>) EPSC modulation at different numbers of pulses (<span class="html-italic">T</span> = 2 s, <span class="html-italic">P</span><sub>inc</sub> = 0.2 mW/cm<sup>2</sup>, <span class="html-italic">V</span><sub>gs</sub> = 0 V, and <span class="html-italic">V</span><sub>ds</sub> = 10 V). (<b>e</b>) Variation in the SNDP ratio with the number of spikes. (<b>f</b>) Synaptic weight decay curves at different pulse numbers with normalized channel conductance at the final spike.</p>
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<p>(<b>a</b>) Schematic of the AZO synaptic transistor operating with a blue LED. (<b>b</b>) EPSC (<span class="html-italic">V</span><sub>gs</sub> = 0 V, <span class="html-italic">V</span><sub>ds</sub> = 10 V, and <span class="html-italic">f</span> = 2.5 Hz) at different numbers of blue LED pulses, a presynaptic optical spike. (<b>c</b>) EPSC is induced by a pair of optical blue LED pulses at an interval time of 500 ms (<span class="html-italic">V</span><sub>gs</sub> = 0 V, <span class="html-italic">V</span><sub>ds</sub> = 10 V). (<b>d</b>) Paired pulse facilitation (PPF) index (<span class="html-italic">V</span><sub>gs</sub> = 0 V, <span class="html-italic">V</span><sub>ds</sub> = 10 V) as a function of optical pulse interval (Δt) with a pulse width of 500 ms. (<b>e</b>) EPSC (<span class="html-italic">V</span><sub>gs</sub> = 0 V, <span class="html-italic">V</span><sub>ds</sub> = 20 V) at a frequency of 0.1–4 Hz with a duration of 200 ms. (<b>f</b>) EPSC gain (A<sub>10</sub>/A<sub>1</sub>). (<b>g</b>) EPSC at different durations for a single pulse (<span class="html-italic">V</span><sub>gs</sub> = 0 V, <span class="html-italic">V</span><sub>ds</sub> = 10 V). (<b>h</b>) Energy consumption at different durations.</p>
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18 pages, 4496 KiB  
Article
Estimation of Aerosol Characteristics from Broadband Solar Radiation Measurements Carried Out in Southern Algeria
by Mohamed Zaiani, Abdanour Irbah and Julien Delanoë
Remote Sens. 2024, 16(18), 3365; https://doi.org/10.3390/rs16183365 - 10 Sep 2024
Viewed by 235
Abstract
Aerosols in the atmosphere significantly reduce the solar radiation reaching the Earth’s surface through scattering and absorption processes. Knowing their properties becomes essential when we are interested in measuring solar radiation at a given location on the ground. The commonly used parameters that [...] Read more.
Aerosols in the atmosphere significantly reduce the solar radiation reaching the Earth’s surface through scattering and absorption processes. Knowing their properties becomes essential when we are interested in measuring solar radiation at a given location on the ground. The commonly used parameters that characterize their effects are the Aerosol Optical Depth τ, the Angstrom exponent α, and the Angstrom coefficient β. One method for estimating these parameters is to fit ground-based measurements of clear-sky direct solar radiation using a model on which it depends. However, the choice of model depends on its suitability to the atmospheric conditions of the site considered. Eleven empirical solar radiation models depending on α and β were thus chosen and tested with solar radiation measurements recorded between 2005 and 2014 in Tamanrasset in southern Algeria. The results obtained were compared to measurements made with the AERONET solar photometer on the same site during the same period. Among the 11 models chosen, the best performing ones are REST2 and CPCR2. They proved to be the best suited to estimate β with approximately the same RMSE of 0.05 and a correlation coefficient R with respect to AERONET of 0.95. The results also highlighted good performances of these models for the estimation of τ with an RMSE of 0.05 and 0.04, and an R of 0.95 and 0.96, respectively. The values of α obtained from the fitting of these models were, however, less good, with R around 0.38. Additional treatments based on a Recurrent Neural Network (RNN) were necessary to improve its estimation. They provided promising results showing a significant improvement in α estimates with R reaching 0.7 when referring to AERONET data. Furthermore, this parameter made it possible to identify different types of aerosols in Tamanrasset such as the presence of maritime, dust, and mixed aerosols representing, respectively, 31.21%, 3.25%, and 65.54%, proportions calculated over the entire period studied. The seasonal analysis showed that maritime aerosols are predominant in the winter in Tamanrasset but decrease with the seasons to reach a minimum in the summer (JJA). Dust aerosols appear in February and persist mainly in the spring (MAM) and summer (JJA), then disappear in September. These results are also consistent with those obtained from AERONET. Full article
(This article belongs to the Special Issue Assessment of Solar Energy Based on Remote Sensing Data)
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Figure 1
<p>(<b>Left</b>): Tamanrasset location. (<b>Right</b>): radiometric station for measuring the global, direct, and diffuse solar radiation: (1) Pyranometer for measuring the global solar irradiance. (2) Pyranometer for measuring the diffuse irradiance component. (3) Peryheliometer for measuring the direct irradiance component. (4) The ball is used to permanently hide the pyranometer (2). (5) The two-axis solar tracker.</p>
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<p>Diagram of creating the predicted model.</p>
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<p>Histograms of Angstrom coefficients (<math display="inline"><semantics> <mi>β</mi> </semantics></math>) obtained with the 11 models from direct solar radiation measurements recorded during the period 2005–2014. The histogram of AERONET <math display="inline"><semantics> <mi>β</mi> </semantics></math> measurements made on the same site and during the same period is also plotted on the bottom-right.</p>
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<p>(<b>Left</b>): temporal variation of Angstrom coefficient <math display="inline"><semantics> <mi>β</mi> </semantics></math> obtained from radiometric (red line) and AERONET (black line) measurements. (<b>Right</b>): correlation between daily values of Angstrom coefficient estimated using clear-sky models and AERONET.</p>
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<p>(<b>Left</b>): temporal variation of the Angstrom exponent <math display="inline"><semantics> <mi>α</mi> </semantics></math> from radiometric (red) and AERONET (black) measurements. (<b>Right</b>): correlation between daily values of Angstrom exponent obtained from AERONET and estimated using three clear-sky models.</p>
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<p>(<b>Left</b>): Angstrom exponent <math display="inline"><semantics> <mi>α</mi> </semantics></math> measured by AERONET (black line) superposed to that estimated from radiometric data using the model CPCR2 (red line). (<b>Right</b>): the same plot with <math display="inline"><semantics> <mi>α</mi> </semantics></math> obtained with the model predicted with RNN (red line).</p>
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<p>Monthly average of estimated Angstrom coefficients (<math display="inline"><semantics> <mi>β</mi> </semantics></math>) for the period 2005–2014 superposed to those obtained from AERONET.</p>
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<p>Predicted Angstrom exponent using 1- (<b>left</b>) and 2-year (<b>right</b>) periods in AERONET dataset for training.</p>
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<p>Regression of estimated <math display="inline"><semantics> <mi>α</mi> </semantics></math> with the measured one when using 1 (<b>left</b>) and 2 (<b>right</b>) years of AERONET data in training.</p>
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<p>AOD <math display="inline"><semantics> <mi>τ</mi> </semantics></math> estimated using direct solar radiation (red) superimposed to AERONET <math display="inline"><semantics> <mi>τ</mi> </semantics></math> measurements (black) for each AERONET wavelength.</p>
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<p>AOD <math display="inline"><semantics> <mi>τ</mi> </semantics></math> estimated from the CPCR2-RNN models using direct solar radiation versus <math display="inline"><semantics> <mi>τ</mi> </semantics></math> measured with AERONET: the regression lines (red) allow the calculation of statistical errors and the correlation factor R.</p>
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<p>(<b>Left</b>): estimated BAOD <math display="inline"><semantics> <msub> <mi>τ</mi> <mrow> <mi>B</mi> <mi>A</mi> <mi>O</mi> <mi>D</mi> </mrow> </msub> </semantics></math> obtained from direct solar radiation measurements (red) superposed to that from AERONET (black). (<b>Right</b>): correlation between <math display="inline"><semantics> <msub> <mi>τ</mi> <mrow> <mi>B</mi> <mi>A</mi> <mi>O</mi> <mi>D</mi> </mrow> </msub> </semantics></math> estimated with CPCR2 model using radiometric measurements and from AERONET.</p>
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<p>Identification of aerosol types in Tamanrasset.</p>
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<p>Monthly (<b>top</b>) and seasonal (<b>bottom</b>) occurrences of identified aerosol types in Tamanrasset.</p>
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12 pages, 1753 KiB  
Article
System Structural Error Analysis in Binocular Vision Measurement Systems
by Miao Yang, Yuquan Qiu, Xinyu Wang, Jinwei Gu and Perry Xiao
J. Mar. Sci. Eng. 2024, 12(9), 1610; https://doi.org/10.3390/jmse12091610 - 10 Sep 2024
Viewed by 167
Abstract
A binocular stereo vision measurement system is widely used in fields such as industrial inspection and marine engineering due to its high accuracy, low cost, and ease of deployment. An unreasonable structural design can lead to difficulties in image matching and inaccuracies in [...] Read more.
A binocular stereo vision measurement system is widely used in fields such as industrial inspection and marine engineering due to its high accuracy, low cost, and ease of deployment. An unreasonable structural design can lead to difficulties in image matching and inaccuracies in depth computation during subsequent processing, thereby limiting the system’s performance and applicability. This paper establishes a systemic error analysis model to enable the validation of changes in structural parameters on the performance of the binocular vision measurement. Specifically, the impact of structural parameters such as baseline distance and object distance on measurement error is analyzed. Extensive experiments reveal that when the ratio of baseline length to object distance is between 1 and 1.5, and the angle between the baseline and the optical axis is between 30 and 40 degrees, the system measurement error is minimized. The experimental conclusions provide guidance for subsequent measurement system research and parameter design. Full article
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Figure 1
<p>A structural model of a binocular vision measurement system.</p>
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<p>An overhead view of the binocular vision system architecture.</p>
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<p>The distribution curve of the systematic error for parameter <math display="inline"><semantics> <mstyle scriptlevel="0" displaystyle="true"> <mi>K</mi> </mstyle> </semantics></math>.</p>
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<p>Variation curve of systematic error relative to external camera parameter error. (<b>a</b>) Distribution curve of systematic error with respect to angle between baseline and optical axis; (<b>b</b>) variation curve of systematic error relative to baseline length.</p>
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<p>Total error distribution curve of system structural parameters.</p>
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<p>System structure.</p>
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<p>Experimental setup.</p>
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<p>Impact of <math display="inline"><semantics> <mstyle scriptlevel="0" displaystyle="true"> <mi>Z</mi> </mstyle> </semantics></math> on systematic error at different <math display="inline"><semantics> <mstyle scriptlevel="0" displaystyle="true"> <mi>B</mi> </mstyle> </semantics></math>.</p>
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<p>Impact of <math display="inline"><semantics> <mstyle scriptlevel="0" displaystyle="true"> <mi>B</mi> </mstyle> </semantics></math> on systematic error at different <math display="inline"><semantics> <mstyle scriptlevel="0" displaystyle="true"> <mi>Z</mi> </mstyle> </semantics></math>.</p>
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<p>Plan view of experimental apparatus.</p>
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<p>Measurement error curves of angle <math display="inline"><semantics> <mstyle scriptlevel="0" displaystyle="true"> <mi>α</mi> </mstyle> </semantics></math> between baseline and optical axis.</p>
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8 pages, 2418 KiB  
Article
A Crack Detection Method for an Insulator Based on the Optical Frequency Domain Reflectometry Fiber Sensing System
by Jing Zhao, Yongqiang Wen, Aodi Yu, Wei Li and Li Xia
Photonics 2024, 11(9), 854; https://doi.org/10.3390/photonics11090854 - 10 Sep 2024
Viewed by 198
Abstract
In this paper, a method for detection of crack locations and the width of basin insulators is proposed. Based on the optical frequency domain reflectometry (OFDR) system, the system utilizes an FBG with high feedback for strain as well as temperature, which is [...] Read more.
In this paper, a method for detection of crack locations and the width of basin insulators is proposed. Based on the optical frequency domain reflectometry (OFDR) system, the system utilizes an FBG with high feedback for strain as well as temperature, which is affixed to the surface of the tub insulator, and a common single-mode optical fiber, which is used for transmitting data and connected to the optical backscattering reflectometry interrogator. The interrogator measures the backscattered light from the FBG, which varies with temperature or strain. The method has been used to measure the location and width of several different cracks and can locate the crack position with a spatial resolution of 1 mm and measure the crack width with a resolution of 0.77 mm. The method has been used to measure the position and width of insulators. This method provides a simple and fast approach to crack detection in insulators. Full article
(This article belongs to the Special Issue Progress and Prospects in Optical Fiber Sensing)
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<p>Schematic diagram (1: potted insulator, 2: FBG, 3 single-mode fiber, 4: OSI interrogator, 5: Type-C cable, 6: laptop).</p>
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<p>Physical diagram of equal strength beam.</p>
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<p>(<b>a</b>): Strain in a 3 mm crack strength beam; (<b>b</b>) strain corresponding to cracks of different sizes; (<b>c</b>) relationship between half-width of strain values and crack widths.</p>
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<p>(<b>a</b>): Schematic of the insulator upper surface; (<b>b</b>): strain values of the insulator upper surface after heating in the crack-free condition.</p>
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<p>(<b>a</b>): Strain values at the cracks of insulators with cracks during heating; (<b>b</b>): strain values at the cracks of insulators with cracks after heating and resting for ten minutes.</p>
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16 pages, 8157 KiB  
Article
Evaluation and Validation on Sensitivity of Near-Infrared Diffuse Reflectance in Non-Invasive Human Blood Glucose Measurement
by Qing Ge, Tongshuai Han, Rong Liu, Zengfu Zhang, Di Sun, Jin Liu and Kexin Xu
Sensors 2024, 24(18), 5879; https://doi.org/10.3390/s24185879 - 10 Sep 2024
Viewed by 198
Abstract
In non-invasive blood glucose measurement, the sensitivity of glucose-induced optical signals within human tissue is a crucial reference point. This study evaluates the sensitivity of glucose-induced diffuse reflectance in the 1000–1700 nm range. A key factor in understanding this sensitivity is the rate [...] Read more.
In non-invasive blood glucose measurement, the sensitivity of glucose-induced optical signals within human tissue is a crucial reference point. This study evaluates the sensitivity of glucose-induced diffuse reflectance in the 1000–1700 nm range. A key factor in understanding this sensitivity is the rate at which the scattering coefficient changes due to glucose, as it is significantly higher than in non-living media and predominantly influences the diffuse light signal level when blood glucose levels change. The study measured and calculated the changes in the scattering coefficient at 1314 nm, a wavelength chosen for its minimal interference from glucose absorption and other bodily constituents. Based on the Mie scattering theory and the results at 1314 nm, the changes in the scattering coefficient within the 1000–1700 nm range were estimated. Subsequently, the sensitivity of the glucose signal across this range was determined through Monte Carlo (MC) simulations. The findings from 25 human trials indicate that the measured sensitivities at five other typical wavelengths within this band generally align with the sensitivities calculated using the aforementioned method. This research can guide the identification of blood glucose signals and the selection of wavelengths for non-invasive blood glucose measurements. Full article
(This article belongs to the Special Issue IMU and Innovative Sensors for Healthcare)
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<p>(<b>a</b>) Linear fitting curve of <math display="inline"><semantics> <mrow> <mi>A</mi> <mo>(</mo> <msub> <mrow> <mi>r</mi> </mrow> <mrow> <mi mathvariant="normal">A</mi> </mrow> </msub> <mo>)</mo> </mrow> </semantics></math> as a function of <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>μ</mi> </mrow> <mrow> <mi mathvariant="normal">s</mi> </mrow> </msub> </mrow> </semantics></math> at 1314 nm. (<b>b</b>) Linear fitting curve of <math display="inline"><semantics> <mrow> <mi>A</mi> <mo>(</mo> <msub> <mrow> <mi>r</mi> </mrow> <mrow> <mi mathvariant="normal">B</mi> </mrow> </msub> <mo>)</mo> </mrow> </semantics></math> as a function of <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>μ</mi> </mrow> <mrow> <mi mathvariant="normal">s</mi> </mrow> </msub> </mrow> </semantics></math> at 1314 nm.</p>
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<p>Block diagram of the experiment system [<a href="#B8-sensors-24-05879" class="html-bibr">8</a>].</p>
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<p>(<b>a</b>) The differential absorbance (A<sub>D</sub>) of the 1314 nm and the glucose reference value (Cg). (<b>b</b>) The fitted line of A<sub>D</sub> and Cg, with the correlation coefficient R between them. (<b>c</b>) Scattering coefficient variation per unit glucose concentration change <math display="inline"><semantics> <mrow> <mstyle scriptlevel="0" displaystyle="true"> <mfrac> <mrow> <mi mathvariant="normal">d</mi> <msub> <mrow> <mi>μ</mi> </mrow> <mrow> <mi mathvariant="normal">s</mi> </mrow> </msub> </mrow> <mrow> <mi mathvariant="normal">d</mi> <msub> <mrow> <mi>C</mi> </mrow> <mrow> <mi mathvariant="normal">g</mi> </mrow> </msub> </mrow> </mfrac> </mstyle> </mrow> </semantics></math> in the 1000–1700 nm range.</p>
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<p>Variation in absorption coefficient due to per unit glucose concentration change <math display="inline"><semantics> <mrow> <mstyle scriptlevel="0" displaystyle="true"> <mfrac> <mrow> <mi mathvariant="normal">d</mi> <msub> <mrow> <mi>μ</mi> </mrow> <mrow> <mi>a</mi> </mrow> </msub> </mrow> <mrow> <mi mathvariant="normal">d</mi> <msub> <mrow> <mi>C</mi> </mrow> <mrow> <mi mathvariant="normal">g</mi> </mrow> </msub> </mrow> </mfrac> </mstyle> </mrow> </semantics></math>.</p>
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<p>(<b>a</b>) <math display="inline"><semantics> <mrow> <mstyle scriptlevel="0" displaystyle="true"> <mfrac> <mrow> <mo>∂</mo> <mi>A</mi> </mrow> <mrow> <mo>∂</mo> <msub> <mrow> <mi>μ</mi> </mrow> <mrow> <mi mathvariant="normal">a</mi> </mrow> </msub> </mrow> </mfrac> </mstyle> </mrow> </semantics></math> obtained by MC simulation, and (<b>b</b>) <math display="inline"><semantics> <mrow> <mstyle scriptlevel="0" displaystyle="true"> <mfrac> <mrow> <mo>∂</mo> <mi>A</mi> </mrow> <mrow> <mo>∂</mo> <msub> <mrow> <mi>μ</mi> </mrow> <mrow> <mi mathvariant="normal">s</mi> </mrow> </msub> </mrow> </mfrac> </mstyle> </mrow> </semantics></math> obtained by MC simulation. (<b>c</b>) The absorbance sensitivity due to glucose’s absorption change, (<b>d</b>) the absorbance sensitivity due to glucose’s scattering change, and (<b>e</b>) the absorbance sensitivity at five SDSs from the calculation results.</p>
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<p>Results of human experiments compared with the calculated results. (<b>a</b>–<b>d</b>) The change in differential absorbance <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>A</mi> </mrow> <mrow> <mi mathvariant="normal">D</mi> </mrow> </msub> </mrow> </semantics></math> from 4 volunteers at the six wavelengths and the glucose reference value (Cg); (<b>e</b>) the experimental sensitivity <math display="inline"><semantics> <mrow> <mstyle scriptlevel="0" displaystyle="true"> <mfrac> <mrow> <mi mathvariant="normal">d</mi> <msub> <mrow> <mi>A</mi> </mrow> <mrow> <mi mathvariant="normal">D</mi> </mrow> </msub> </mrow> <mrow> <mi mathvariant="normal">d</mi> <msub> <mrow> <mi>C</mi> </mrow> <mrow> <mi mathvariant="normal">g</mi> </mrow> </msub> </mrow> </mfrac> </mstyle> </mrow> </semantics></math> of all 25 cases; (<b>f</b>) calculated and average experimental sensitivity <math display="inline"><semantics> <mrow> <mstyle scriptlevel="0" displaystyle="true"> <mfrac> <mrow> <mi mathvariant="normal">d</mi> <msub> <mrow> <mi>A</mi> </mrow> <mrow> <mi mathvariant="normal">D</mi> </mrow> </msub> </mrow> <mrow> <mi mathvariant="normal">d</mi> <msub> <mrow> <mi>C</mi> </mrow> <mrow> <mi mathvariant="normal">g</mi> </mrow> </msub> </mrow> </mfrac> </mstyle> </mrow> </semantics></math> of 25 cases.</p>
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<p>Results of sensitivity calculations in intralipid solution: (<b>a</b>) variation of sensitivity with wavelength at different source–detector separations; (<b>b</b>) impact of glucose–induced absorption changes on sensitivity; (<b>c</b>) impact of glucose-induced scattering changes on sensitivity.</p>
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<p>(<b>a</b>) Glucose detection sensitivity of differential absorbance for male and female skin; (<b>b</b>) glucose detection sensitivity of differential absorbance for elderly and young skin; and (<b>c</b>) glucose detection sensitivity of differential absorbance among the four groups of subjects at wavelengths of 1550 nm and 1609 nm.</p>
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25 pages, 6231 KiB  
Article
Physical Properties of an Efficient MAPbBr3/GaAs Hybrid Heterostructure for Visible/Near-Infrared Detectors
by Tarek Hidouri, Maura Pavesi, Marco Vaccari, Antonella Parisini, Nabila Jarmouni, Luigi Cristofolini and Roberto Fornari
Nanomaterials 2024, 14(18), 1472; https://doi.org/10.3390/nano14181472 - 10 Sep 2024
Viewed by 181
Abstract
Semiconductor photodetectors can work only in specific material-dependent light wavelength ranges, connected with the bandgaps and absorption capabilities of the utilized semiconductors. This limitation has driven the development of hybrid devices that exceed the capabilities of individual materials. In this study, for the [...] Read more.
Semiconductor photodetectors can work only in specific material-dependent light wavelength ranges, connected with the bandgaps and absorption capabilities of the utilized semiconductors. This limitation has driven the development of hybrid devices that exceed the capabilities of individual materials. In this study, for the first time, a hybrid heterojunction photodetector based on methylammonium lead bromide (MAPbBr3) polycrystalline film deposited on gallium arsenide (GaAs) was presented, along with comprehensive morphological, structural, optical, and photoelectrical investigations. The MAPbBr3/GaAs heterojunction photodetector exhibited wide spectral responsivity, from 540 to 900 nm. The fabrication steps of the prototype device, including a new preparation recipe for the MAPbBr3 solution and spinning, will be disclosed and discussed. It will be shown that extending the soaking time and refining the precursor solution’s stoichiometry may enhance surface coverage, adhesion to the GaAs, and film uniformity, as well as provide a new way to integrate MAPbBr3 on GaAs. Compared to the pristine MAPbBr3, the enhanced structural purity of the perovskite on GaAs was confirmed by X-ray Diffraction (XRD) upon optimization compared to the conventional glass substrate. Scanning Electron Microscopy (SEM) revealed the formation of microcube-like structures on the top of an otherwise continuous MAPbBr3 polycrystalline film, with increased grain size and reduced grain boundary effects pointed by Energy-Dispersive Spectroscopy (EDS) and cathodoluminescence (CL). Enhanced absorption was demonstrated in the visible range and broadened photoluminescence (PL) emission at room temperature, with traces of reduction in the orthorhombic tilting revealed by temperature-dependent PL. A reduced average carrier lifetime was reduced to 13.8 ns, revealed by time-resolved PL (TRPL). The dark current was typically around 8.8 × 10−8 A. Broad photoresponsivity between 540 and 875 nm reached a maximum of 3 mA/W and 16 mA/W, corresponding to a detectivity of 6 × 1010 and 1 × 1011 Jones at −1 V and 50 V, respectively. In case of on/off measurements, the rise and fall times were 0.40 s and 0.61 s or 0.62 s and 0.89 s for illumination, with 500 nm or 875 nm photons, respectively. A long-term stability test at room temperature in air confirmed the optical and structural stability of the proposed hybrid structure. This work provides insights into the physical mechanisms of new hybrid junctions for high-performance photodetectors. Full article
(This article belongs to the Special Issue Physical Properties of Semiconductor Nanostructures and Devices)
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<p>Schematic presentation of the multistep process for the deposition of MAPbBr<sub>3</sub> on GaAs. Acronyms of the chemical compounds are provided in the article text.</p>
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<p>(<b>a</b>) XRD spectrum of MAPbBr<sub>3</sub>/GaAs (sample S *, see <a href="#nanomaterials-14-01472-t001" class="html-table">Table 1</a>) with a zoomed portion of the spectrum to highlight the MAPbBr<sub>3</sub> peaks; (<b>b</b>) SEM images showing poor (upper image) and improved coverage (lower image) by the perovskite microcubes and the formation of an underlying layer (red circles).</p>
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<p>(<b>a</b>) Top-view SEM images showing the effect of the antisolvent soaking time on the morphology of MAPbBr<sub>3</sub>/GaAs, with reference to <a href="#nanomaterials-14-01472-t001" class="html-table">Table 1</a> (image 1, sample S *); (image 2, sample S1); (image 3, sample S2); (image 4, sample S3); and (image 5, sample S4). The corresponding insets are photos of the sample surfaces. (<b>b</b>) Top-view and cross-section SEM of S4 (image 5) with 1 cm<sup>2</sup> full surface coverage, as seen in the surface photo in the inset; (<b>c</b>) XRD diffractogram of S4.</p>
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<p>Typical energy-dispersive X-ray spectroscopy (EDX) elemental mapping images showing the EDS layered image of S4 and corresponding element analysis.</p>
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<p>SEM-CL images of the MAPbBr<sub>3</sub>/GaAs heterostructure (sample S4). (<b>a</b>) The original CL image. (<b>b</b>,<b>c</b>) Treated SEM-CL images for better clarity.</p>
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<p>(<b>a</b>) Absorption spectra; (<b>b</b>) PL spectra taken at 300 K, showing that the broad MAPbBr<sub>3</sub>/GaAs emission is deconvoluted using the Gaussian function (dashed green lines); (<b>c</b>) power-dependent PL spectra of MAPbBr<sub>3</sub>/GaAs; inset shows the power-dependent PL spectra of the control (S0 *); (<b>d</b>) integrated PL intensity vs. excitation power (black dots) fitted with power law (red solid line); (<b>e</b>) time-resolved PL spectra of the control (S0 *) and MAPbBr<sub>3</sub>/GaAs (S4), showing the experimental time trace (dots) with bi-exponential fit (solid lines) at a fixed density of excited carriers; (<b>f</b>) time-resolved PL spectra of MAPbBr<sub>3</sub>/GaAs (sample S4) acquired at different densities of excited carriers (different photon density) and the corresponding time constants, using bi-exponential fit.</p>
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<p>(<b>a</b>) Absorption spectra; (<b>b</b>) PL spectra taken at 300 K, showing that the broad MAPbBr<sub>3</sub>/GaAs emission is deconvoluted using the Gaussian function (dashed green lines); (<b>c</b>) power-dependent PL spectra of MAPbBr<sub>3</sub>/GaAs; inset shows the power-dependent PL spectra of the control (S0 *); (<b>d</b>) integrated PL intensity vs. excitation power (black dots) fitted with power law (red solid line); (<b>e</b>) time-resolved PL spectra of the control (S0 *) and MAPbBr<sub>3</sub>/GaAs (S4), showing the experimental time trace (dots) with bi-exponential fit (solid lines) at a fixed density of excited carriers; (<b>f</b>) time-resolved PL spectra of MAPbBr<sub>3</sub>/GaAs (sample S4) acquired at different densities of excited carriers (different photon density) and the corresponding time constants, using bi-exponential fit.</p>
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<p>(<b>a</b>) Temperature dependence of the PL emission energy of the high-energy peak of MAPbBr<sub>3</sub>/GaAs (S4) (red dots) and its control sample (blue dots). (<b>b</b>) Temperature-dependent PL intensity of MAPbBr<sub>3</sub>/GaAs (red dots) fitted by Arrhenius law.</p>
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<p>Structural, optical, and cycling stability of the MAPbBr<sub>3</sub>/GaAs heterojunction (sample S4).</p>
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<p>Structural, optical, and cycling stability of the MAPbBr<sub>3</sub>/GaAs heterojunction (sample S4).</p>
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<p>(<b>a</b>) I–V response in semi-log scale in the dark (black symbols) and under 500 nm light illumination (blue symbols). (<b>b</b>) Room-temperature dark forward current–voltage characteristics in a semi-log scale. The linear fitting (red solid line) of ln(I)–V is shown. Inset: the obtained ideality factor extracted from the low-injection region.</p>
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<p>(<b>a</b>) I–V response in semi-log scale in the dark (black symbols) and under 500 nm light illumination (blue symbols). (<b>b</b>) Room-temperature dark forward current–voltage characteristics in a semi-log scale. The linear fitting (red solid line) of ln(I)–V is shown. Inset: the obtained ideality factor extracted from the low-injection region.</p>
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<p>(<b>a</b>) Schematic energy band diagrams of the junction (S4) under illumination and reverse bias. (<b>b</b>) Schematic design of the final device and (<b>c</b>) the extracted responsivity and detectivity under 500 nm illumination and bias of −1 V.</p>
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<p>(<b>a</b>) Responsivity of MAPbBr<sub>3</sub>/GaAs under −0.5 V (green symbols) and −1 V (black symbols) for illumination with 500 nm photons. (<b>b</b>) Time-dependent photoresponse showing the on/off switching cycles for 500 nm illumination at −1 V of the sample S4 (red dots) and the control sample S * (blue dots). (<b>c</b>) Time-dependent photoresponse of MAPbBr<sub>3</sub>/GaAs under 500 nm and 875 nm illumination at a constant bias (−1 V).</p>
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13 pages, 5329 KiB  
Article
Performance Properties and Finite Element Modelling of Forest-Based Bionanomaterials/Activated Carbon Composite Film for Sustainable Future
by Mustafa Zor, Ferhat Şen, Orhan Özçelik, Hikmet Yazıcı and Zeki Candan
Forests 2024, 15(9), 1591; https://doi.org/10.3390/f15091591 - 10 Sep 2024
Viewed by 187
Abstract
Thanks to its highly crystalline structure and excellent thermal, optical, electrical and mechanical properties, carbon and its derivatives are considered the preferred reinforcement material in composites used in many industrial applications, especially in the forest and forest products sector, including oil, gas and [...] Read more.
Thanks to its highly crystalline structure and excellent thermal, optical, electrical and mechanical properties, carbon and its derivatives are considered the preferred reinforcement material in composites used in many industrial applications, especially in the forest and forest products sector, including oil, gas and aviation. Since hydroxyethyl cellulose (HEC) is a biopolymer, it has poor mechanical and thermal properties. These properties need to be strengthened with various additives. This study aims to improve the thermal and mechanical properties of hydroxyethyl cellulose by preparing hydroxyethyl cellulose/activated carbon (HEC/AC) composite materials. With this study, composites were obtained for the first time and their mechanical properties were examined using a 3D numerical modeling technique. The thermal stability of the prepared composite materials was investigated via thermal gravimetric analysis (TGA). The samples were heated from 30 °C to 750 °C with a heating rate of 10 °C/min under a nitrogen atmosphere and their masses were measured subsequently. The mechanical properties of the composites were investigated via the tensile test. The viscoelastic properties of the composite films were determined with dynamic mechanical thermal analyses (DMTA) and their morphologies were examined with scanning electron microscopy (SEM) images. According to the results, the best F3 sample (films containing 3 wt.% activated carbon) had an elastic modulus of 168.3 MPa, a thermal conductivity value of 0.068 W/mK, the maximum mass loss was at 328.20 °C and the initial storage modulus at 30 °C was 206.13 MPa. It was determined that the hydroxyethyl cellulose composite films containing 3 wt.% activated carbon revealed the optimum results in terms of both thermal conductivity and viscoelastic response and showed that the obtained composite films could be used in industrial applications where thermal conductivity was required. Full article
(This article belongs to the Special Issue Sustainable Materials in the Forest Products Industry)
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<p>Random particle RVE for HEC/AC composite films with 1 wt.% activated carbon (F2): (<b>a</b>) RVE with randomly distributed particles, (<b>b</b>) finite element mesh of the RVE.</p>
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<p>Random particle RVE for HEC/AC composite films with 3 wt.% activated carbon (F3): (<b>a</b>) RVE with randomly distributed particles, (<b>b</b>) finite element mesh of the RVE.</p>
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<p>Random particle RVE for HEC/AC composite films with 5 wt.% activated carbon (F4): (<b>a</b>) RVE with randomly distributed particles, (<b>b</b>) finite element mesh of the RVE.</p>
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<p>Stress vs. strain curves of neat HEC and HEC/AC composite films.</p>
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<p>The distribution of axial normal stress in HEC/AC with 5 wt.% AC (F4) in tensile test at 4% strain.</p>
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<p>Thermal conductivity of the composite films.</p>
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<p>TGA/DTG of the composite films.</p>
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<p>Dynamic mechanical analysis of the composite films.</p>
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<p>SEM images of the composite films (Arrows indicate activated carbon particles).</p>
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12 pages, 3246 KiB  
Article
Mechanism of Improving Etching Selectivity for E-Beam Resist AR-N 7520 in the Formation of Photonic Silicon Structures
by Ksenia Fetisenkova, Alexander Melnikov, Vitaly Kuzmenko, Andrey Miakonkikh, Alexander Rogozhin, Andrey Tatarintsev, Oleg Glaz and Vsevolod Kiselevsky
Processes 2024, 12(9), 1941; https://doi.org/10.3390/pr12091941 - 10 Sep 2024
Viewed by 195
Abstract
The selectivity of the reactive ion etching of silicon using a negative electron resist AR-N 7520 mask was investigated. The selectivity dependencies on the fraction of SF6 in the feeding gas and bias voltage were obtained. To understand the kinetics of passivation [...] Read more.
The selectivity of the reactive ion etching of silicon using a negative electron resist AR-N 7520 mask was investigated. The selectivity dependencies on the fraction of SF6 in the feeding gas and bias voltage were obtained. To understand the kinetics of passivation film formation and etching, the type and concentration of neutral particles were evaluated and identified using plasma optical emission spectroscopy. Electron temperature and electron density were measured by the Langmuir probe method to interpret the optical emission spectroscopy data. A high etching selectivity of 8.0 ± 1.8 was obtained for the etching process. The optimum electron beam exposure dose for defining the mask was 8200 pC/m at 30 keV. Full article
(This article belongs to the Section Manufacturing Processes and Systems)
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<p>(<b>a</b>–<b>c</b>) SEM images of samples after development. Lines with exposure doses of (<b>a</b>) 4000 pC/cm, (<b>b</b>) 5800 pC/cm, and (<b>c</b>) 8200 pC/cm are presented. (<b>d</b>) Dependence of line height after development on the line exposure dose.</p>
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<p>Dependence of line edge roughness (LER) on exposure dose.</p>
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<p>(<b>a</b>) Plasma spectrum of the SF<sub>6</sub>/C<sub>4</sub>F<sub>8</sub> feeding gas composition under experimental conditions with the SF<sub>6</sub> fraction equal to 18%. The fraction of Ar is equal to 6%. (<b>b</b>) Spectrum of molecular bands and CF<sub>x</sub> continuum in the ultraviolet region for SF<sub>6</sub>/C<sub>4</sub>F<sub>8</sub> plasma under experimental conditions.</p>
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<p>Dependence of atomic fluorine concentration and intensity of the overlapped CF<sub>2</sub> molecular bands A<sup>1</sup>B<sub>1</sub>(0;3;0)–X<sup>1</sup>A<sub>1</sub>(0;0;0) and A<sup>1</sup>B<sub>1</sub>(0;4;0)–X<sup>1</sup>A<sub>1</sub>(0;1;0) (262.5 nm) on the SF<sub>6</sub> fraction in the feeding gas.</p>
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<p>(<b>a</b>–<b>e</b>) SEM images of samples after the process of RIE. Structures after processes with SF<sub>6</sub> fractions of (<b>a</b>) 15%, (<b>b</b>) 18%, (<b>c</b>) 25%, (<b>d</b>) 28%, and (<b>e</b>) 31%. (<b>f</b>) Dependence of silicon-etching rate, the etching rate of AR-N 7520, and selectivity on the SF<sub>6</sub> fraction in the feeding gas. The mean error values for the silicon and resistetching rates were 5.5 nm/min and 8.5 nm/min, respectively.</p>
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<p>Dependence of silicon-etching rate, the etching rate of AR-N 7520 resist, and selectivity on the bias voltage. The mean error values for the silicon- and resist etching rates were 5.2 nm/min and 10.5 nm/min, respectively.</p>
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<p>Dependence of selectivity on the exposure dose for etching processes with different values of bias voltage.</p>
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<p>Dependence of the silicon structure sidewall angle on the SF<sub>6</sub> fraction in SF<sub>6</sub>/C<sub>4</sub>F<sub>8</sub> feeding gas. SEM images of the structures are shown in <a href="#processes-12-01941-f005" class="html-fig">Figure 5</a>a–e.</p>
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13 pages, 5820 KiB  
Article
Optic Nerve Sheath Ultrasound Image Segmentation Based on CBC-YOLOv5s
by Yonghua Chu, Jinyang Xu, Chunshuang Wu, Jianping Ye, Jucheng Zhang, Lei Shen, Huaxia Wang and Yudong Yao
Electronics 2024, 13(18), 3595; https://doi.org/10.3390/electronics13183595 - 10 Sep 2024
Viewed by 186
Abstract
The diameter of the optic nerve sheath is an important indicator for assessing the intracranial pressure in critically ill patients. The methods for measuring the optic nerve sheath diameter are generally divided into invasive and non-invasive methods. Compared to the invasive methods, the [...] Read more.
The diameter of the optic nerve sheath is an important indicator for assessing the intracranial pressure in critically ill patients. The methods for measuring the optic nerve sheath diameter are generally divided into invasive and non-invasive methods. Compared to the invasive methods, the non-invasive methods are safer and have thus gained popularity. Among the non-invasive methods, using deep learning to process the ultrasound images of the eyes of critically ill patients and promptly output the diameter of the optic nerve sheath offers significant advantages. This paper proposes a CBC-YOLOv5s optic nerve sheath ultrasound image segmentation method that integrates both local and global features. First, it introduces the CBC-Backbone feature extraction network, which consists of dual-layer C3 Swin-Transformer (C3STR) and dual-layer Bottleneck Transformer (BoT3) modules. The C3STR backbone’s multi-layer convolution and residual connections focus on the local features of the optic nerve sheath, while the Window Transformer Attention (WTA) mechanism in the C3STR module and the Multi-Head Self-Attention (MHSA) in the BoT3 module enhance the model’s understanding of the global features of the optic nerve sheath. The extracted local and global features are fully integrated in the Spatial Pyramid Pooling Fusion (SPPF) module. Additionally, the CBC-Neck feature pyramid is proposed, which includes a single-layer C3STR module and three-layer CReToNeXt (CRTN) module. During upsampling feature fusion, the C3STR module is used to enhance the local and global awareness of the fused features. During downsampling feature fusion, the CRTN module’s multi-level residual design helps the network to better capture the global features of the optic nerve sheath within the fused features. The introduction of these modules achieves the thorough integration of the local and global features, enabling the model to efficiently and accurately identify the optic nerve sheath boundaries, even when the ocular ultrasound images are blurry or the boundaries are unclear. The Z2HOSPITAL-5000 dataset collected from Zhejiang University Second Hospital was used for the experiments. Compared to the widely used YOLOv5s and U-Net algorithms, the proposed method shows improved performance on the blurry test set. Specifically, the proposed method achieves precision, recall, and Intersection over Union (IoU) values that are 4.1%, 2.1%, and 4.5% higher than those of YOLOv5s. When compared to U-Net, the precision, recall, and IoU are improved by 9.2%, 21%, and 19.7%, respectively. Full article
(This article belongs to the Special Issue Deep Learning-Based Object Detection/Classification)
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<p>CBC-YOLOv5s optic nerve sheath segmentation algorithm.</p>
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<p>C3STR module.</p>
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<p>BoT3 module.</p>
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<p>CRTN module.</p>
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<p>Different algorithms for visualization with normal and blurry images.</p>
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<p>Different algorithms for segmentation examples with normal and blurry images.</p>
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13 pages, 4429 KiB  
Article
Photo-Thermal Conversion and Raman Sensing Properties of Three-Dimensional Gold Nanostructure
by Feng Shan, Jingyi Huang, Yanyan Zhu and Guohao Wei
Molecules 2024, 29(18), 4287; https://doi.org/10.3390/molecules29184287 - 10 Sep 2024
Viewed by 162
Abstract
Three-dimensional plasma nanostructures with high light–thermal conversion efficiency show the prospect of industrialization in various fields and have become a research hotspot in areas of light–heat utilization, solar energy capture, and so on. In this paper, a simple chemical synthesis method is proposed [...] Read more.
Three-dimensional plasma nanostructures with high light–thermal conversion efficiency show the prospect of industrialization in various fields and have become a research hotspot in areas of light–heat utilization, solar energy capture, and so on. In this paper, a simple chemical synthesis method is proposed to prepare gold nanoparticles, and the electrophoretic deposition method is used to assemble large-area three-dimensional gold nanostructures (3D-GNSs). The light–thermal water evaporation monitoring and surface-enhanced Raman scattering (SERS) measurements of 3D-GNSs were performed via theoretical simulation and experiments. We reveal the physical processes of local electric field optical enhancement and the light–thermal conversion of 3D-GNSs. The results show that with the help of the efficient optical trapping and super-hydrophilic surface properties of 3D-GNSs, they have a significant effect in accelerating water evaporation, which was increased by nearly eight times. At the same time, the three-dimensional SERS substrates based on gold nanosphere particles (GNSPs) and gold nanostar particles (GNSTs) had limited sensitivities of 10−10 M and 10−12 M to R6G molecules, respectively. Therefore, 3D-GNSs show strong competitiveness in the fields of solar-energy-induced water purification and the Raman trace detection of organic molecules. Full article
(This article belongs to the Special Issue Raman Spectroscopy Analysis of Surfaces)
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<p>(<b>a</b>) The absorption spectrum of the gold seed solution (inset: gold seed solution). (<b>b</b>) The TEM image of gold seed nanoparticles.</p>
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<p>SEM images of (<b>a</b>) GNSPs and (<b>b</b>) GNSTs. (<b>c</b>) Absorption spectra of GNSP and GNST solutions.</p>
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<p>Electric field distributions on the surface of (<b>a</b>) a single GNSP and (<b>b</b>) two GNSPs. (<b>c</b>) Electric field resonance spectra on the surface of a single GNSP and two GNSPs. Electric field distributions on the surface of (<b>d</b>) a single GNST and (<b>e</b>) two GNSTs. (<b>f</b>) Local electric field resonance spectra on the surface of a single GNST and two GNSTs.</p>
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<p>(<b>a</b>) Schematic illustration of the electrophoretic deposition method. (<b>b</b>) Experimental equipment used for assembling 3D-GNSs via electrophoretic deposition. (<b>c</b>) Physical picture of 3D-GNSs assembled via electrophoretic deposition.</p>
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<p>SEM images of (<b>a</b>) GNSP films and (<b>b</b>) GNST films. Images of the coupling effect within the electric field distribution for (<b>c</b>) GNSPs and (<b>d</b>) GNSTs. The insets in (<b>a</b>,<b>b</b>) are higher-magnification SEM images.</p>
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<p>(<b>a</b>) EDS spectrum of 3D-GNS. (<b>b</b>) Shape of water droplets on the surface of 3D-GNS. (<b>c</b>) Shape of water droplets on the surface of ITO glass. (<b>d</b>) Water drop contact angle on the 3D-GNS surface. (<b>e</b>) Water drop contact angle on the ITO glass surface. (<b>f</b>) Water droplet evaporation rate on the ITO glass and 3D-GNS surfaces.</p>
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<p>(<b>a</b>) Raman spectra of R6G molecules on 3D-GNS SERS substrate based on GNSPs. (<b>b</b>) Raman spectra of R6G molecules on 3D-GNS SERS substrate based on GNSTs.</p>
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<p>Schematic illustration of the synthesis of GNSTs.</p>
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9 pages, 4539 KiB  
Communication
Fabrication of Circular Defects in 2-Dimensional Photonic Crystal Lasers with Convex Edge Structure
by Rubing Zuo, Yuki Adachi, Yuto Kudo, Hanqiao Ye, Tetsuya Yagi, Masato Morifuji, Hirotake Kajii, Akihiro Maruta and Masahiko Kondow
Photonics 2024, 11(9), 853; https://doi.org/10.3390/photonics11090853 - 10 Sep 2024
Viewed by 163
Abstract
We have developed circular defects in 2-dimensional photonic crystal lasers that allow current injection for interconnected optical communications. However, when cleaving the sample to measure the output light, the output light intensity changes due to the cleaving position. In a previous study, we [...] Read more.
We have developed circular defects in 2-dimensional photonic crystal lasers that allow current injection for interconnected optical communications. However, when cleaving the sample to measure the output light, the output light intensity changes due to the cleaving position. In a previous study, we proposed a new end face structure called a convex edge structure. In this paper, we design the electron beam lithography patterns to fabricate this structure. With this design, it is possible to eliminate the effect of different cleaving positions and ensure that the cleavage tolerance is larger than the cleavage position error. We also develop the fabrication technology for this structure, fabricate samples, and measure the output light experimentally. The optical properties of the fabricated sample are similar to well-fabricated samples with normal cleavage edge faces. We are assured that these results contribute to future work such as accurate manufacturing and improving the end face configuration to obtain higher outputs. Full article
(This article belongs to the Special Issue Photonic Crystals: Physics and Devices, 2nd Edition)
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<p>Schematic of two types of edge structures in CirD lasers: (<b>a</b>) edge produced by conventional cleavage; (<b>b</b>) convex edge structure.</p>
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<p>Designs of EB lithography patterns: (<b>a</b>) convex edge structure with a deep trench; (<b>b</b>) symmetric construction; (<b>c</b>) multiple patterns are lined up in the y direction and shifted in the x direction to increase the cleavage range.</p>
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<p>Designs of EB lithography patterns: (<b>a</b>) convex edge structure with a deep trench; (<b>b</b>) symmetric construction; (<b>c</b>) multiple patterns are lined up in the y direction and shifted in the x direction to increase the cleavage range.</p>
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<p>Fabrication process flow diagram.</p>
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<p>Cross-sectional SEM image of sample with a collapsing contact layer.</p>
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<p>Top-view SEM image of fabricated sample.</p>
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<p>Relationship between input power and output power measured by PD array and monochromator.</p>
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<p>Spectra of a typical sample measured by OSA: (<b>a</b>) input power was 210 µW. (<b>b</b>) input power was 48 µW.</p>
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29 pages, 10785 KiB  
Article
Large-Scale Network-Based Observations of a Saharan Dust Event across the European Continent in Spring 2022
by Christina-Anna Papanikolaou, Alexandros Papayannis, Marilena Gidarakou, Sabur F. Abdullaev, Nicolae Ajtai, Holger Baars, Dimitris Balis, Daniele Bortoli, Juan Antonio Bravo-Aranda, Martine Collaud-Coen, Benedetto de Rosa, Davide Dionisi, Kostas Eleftheratos, Ronny Engelmann, Athena A. Floutsi, Jesús Abril-Gago, Philippe Goloub, Giovanni Giuliano, Pilar Gumà-Claramunt, Julian Hofer, Qiaoyun Hu, Mika Komppula, Eleni Marinou, Giovanni Martucci, Ina Mattis, Konstantinos Michailidis, Constantino Muñoz-Porcar, Maria Mylonaki, Michail Mytilinaios, Doina Nicolae, Alejandro Rodríguez-Gómez, Vanda Salgueiro, Xiaoxia Shang, Iwona S. Stachlewska, Horațiu Ioan Ștefănie, Dominika M. Szczepanik, Thomas Trickl, Hannes Vogelmann and Kalliopi Artemis Voudouriadd Show full author list remove Hide full author list
Remote Sens. 2024, 16(17), 3350; https://doi.org/10.3390/rs16173350 - 9 Sep 2024
Viewed by 323
Abstract
Between 14 March and 21 April 2022, an extensive investigation of an extraordinary Saharan dust intrusion over Europe was performed based on lidar measurements obtained by the European Aerosol Research Lidar Network (EARLINET). The dust episode was divided into two distinct periods, one [...] Read more.
Between 14 March and 21 April 2022, an extensive investigation of an extraordinary Saharan dust intrusion over Europe was performed based on lidar measurements obtained by the European Aerosol Research Lidar Network (EARLINET). The dust episode was divided into two distinct periods, one in March and one in April, characterized by different dust transport paths. The dust aerosol layers were studied over 18 EARLINET stations, examining aerosol characteristics during March and April in four different regions (M-I, M-II, M-III, and M-IV and A-I, A-II, A-III, and A-IV, respectively), focusing on parameters such as aerosol layer thickness, center of mass (CoM), lidar ratio (LR), particle linear depolarization ratio (PLDR), and Ångström exponents (ÅE). In March, regions exhibited varying dust geometrical and optical properties, with mean CoM values ranging from approximately 3.5 to 4.8 km, and mean LR values typically between 36 and 54 sr. PLDR values indicated the presence of both pure and mixed dust aerosols, with values ranging from 0.20 to 0.32 at 355 nm and 0.24 to 0.31 at 532 nm. ÅE values suggested a range of particle sizes, with some regions showing a predominance of coarse particles. Aerosol Optical Depth (AOD) simulations from the NAAPS model indicated significant dust activity across Europe, with AOD values reaching up to 1.60. In April, dust aerosol layers were observed between 3.2 to 5.2 km. Mean LR values typically ranged from 35 to 51 sr at both 355 nm and 532 nm, while PLDR values confirmed the presence of dust aerosols, with mean values between 0.22 and 0.31 at 355 nm and 0.25 to 0.31 at 532 nm. The ÅE values suggested a mixture of particle sizes. The AOD values in April were generally lower, not exceeding 0.8, indicating a less intense dust presence compared to March. The findings highlight spatial and temporal variations in aerosol characteristics across the regions, during the distinctive periods. From 15 to 16 March 2022, Saharan dust significantly reduced UV-B radiation by approximately 14% over the ATZ station (Athens, GR). Backward air mass trajectories showed that the dust originated from the Western and Central Sahara when, during this specific case, the air mass trajectories passed over GRA (Granada, ES) and PAY (Payerne, CH) before reaching ATZ, maintaining high relative humidity and almost stable aerosol properties throughout its transport. Lidar data revealed elevated aerosol backscatter (baer) and PLDR values, combined with low LR and ÅE values, indicative of pure dust aerosols. Full article
(This article belongs to the Section Atmospheric Remote Sensing)
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<p>The EARLINET stations that provided high-quality observations were used in this study. The 3-letter code identifies the station according to the conventions defined within the infrastructure.</p>
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<p>Map of the AOD at 550 nm, calculated by the NAAPS model during March 2022 (period of this study) for three aerosol types: mineral dust (green/yellow), sulfates/ABF (orange/red), and smoke (blue).</p>
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<p>Map of the AOD at 550 nm, calculated by the NAAPS model during April 2022, for three aerosol types: mineral dust (green/yellow), sulfates/ABF (orange/red), and smoke (blue).</p>
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<p>The 168 h backward trajectories of air masses arriving over 4 regions, derived from data collected by 17 lidar stations during March 2022. These trajectories were calculated for air masses arriving at the center altitude of each observed dust layer. The faint colored lines represent the total backward air mass trajectories, while the bold trajectories represent the mean trajectory for each station during the period of March 2022.</p>
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<p>The 168 h backward trajectories of air masses arriving over 4 regions, derived from data collected by the 13 different lidar stations that measured dust aerosol layers during April 2022. These trajectories were calculated for air masses arriving at the center altitude of each observed dust layer. The faint colored lines represent the total backward air mass trajectories, while the bold trajectories represent the mean trajectory for each station during the period of April 2022.</p>
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<p>Observation days and Saharan dust aerosol layers per station for the March (<b>top</b>) and April (<b>bottom</b>) periods, respectively.</p>
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<p>Median, mean, standard deviation, and minimum and maximum values of geometrical and optical properties of the dust aerosol layers observed over each station with measurements during the March period of dust. Differently colored rectangles correspond to the different regions that originated during this period.</p>
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<p>Median, mean, standard deviation, and minimum and maximum values of geometrical and optical properties of the dust aerosol layers observed over each of the stations with measurements during the April period. Differently colored rectangles correspond to the different regions that originated during this period.</p>
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<p>Geometrical and optical properties, mean values, and std obtained per station using the CALIPSO satellite during the dust periods of March and April 2022. Different colored lines correspond to different stations. Missing stations did not provide any layers based on CALIPSO observations.</p>
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<p>The spatio-temporal evolution of the range-corrected lidar signal at 532 nm over Athens on 16 March 2022.</p>
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<p>Daytime evolution of the total UV-B radiation (W/m<sup>2</sup>), along with the SZA (degrees) and the Temperature (°C), reaching the ground, as measured by the Brewer spectrophotometer of BRFAA from 15 to 17 March 2022 over Athens.</p>
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<p>HYSPLIT backward trajectories of the air mass during 15–16 March 2022, ending over (<b>a</b>) the ATZ, (<b>b</b>) PAY, and (<b>c</b>) GRA stations.</p>
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<p>Vertical distribution of the aerosol optical properties (b<sub>aer</sub> at 355 and 532 nm) along with mean values of the PLDR at 355 and 532 nm (blue and green stars) as measured by the three lidar stations (<b>a</b>) GRA, (<b>b</b>) PAY, and (<b>c</b>) ATZ studied in this case study. Light blue and red lines correspond to relative humidity (RH) and temperature (T) obtained by radiosondes for the corresponding day and time of the lidar profiles, provided by the Department of Atmospheric Science, University of Wyoming.</p>
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<p>PM<sub>10</sub>/PM<sub>2.5</sub> ratio within the period of 15–18 March 2022 over the PAY station. The dotted box corresponds to the time period within which the lidar profile lies.</p>
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